NGC 753

{{Short description|Galaxy in the constellation Andromeda}}

{{Sky|01|57|42.2104|+|35|54|58.262}}

{{Infobox Galaxy

| name = NGC 753

| image = PanSTARRS NGC 753.jpg

| caption= NGC 753 imaged by PanSTARRS

| constellation name = Andromeda

| epoch = J2000

| type = SAB(rs)bc{{cite web

| website=NASA/IPAC Extragalactic Database

| publisher = NASA and Caltech

| title=Results for object NGC 0753

| url=https://ned.ipac.caltech.edu/byname?objname=NGC+0753

| access-date=2019-01-03}}

| ra = {{RA|01|57|42.2104}}

| dec = {{DEC|+35|54|58.262}}

| dist_ly = {{convert|67|Mpc|Mly|abbr=on|lk=on|order=flip}}

| z = 0.016221

| h_radial_v = 4863 km/s

| group_cluster = Abell 262

| appmag_v = 12.97

| size_v = {{Val|2.5|×|1.9|u=arcminute}}

| size = ~{{convert|45.39|kpc|ly|abbr=on|lk=on|order=flip}} (estimated)

| names = {{odlist | IRAS= 01547+3540 | MCG= +06-05-066 | PGC= 7387 | UGC= 1437 | CGCG= 522-086}}

}}

NGC 753 is a spiral galaxy located 220 million light-years away{{Cite journal|last1=Pilyugin|first1=L. S.|last2=Grebel|first2=E. K.|last3=Kniazev|first3=A. Y.|date=2014|title=The Abundance Properties of Nearby Late-type Galaxies. I. The Data|url=http://stacks.iop.org/1538-3881/147/i=6/a=131|journal=The Astronomical Journal|language=en|volume=147|issue=6|pages=131|doi=10.1088/0004-6256/147/6/131|issn=1538-3881|bibcode=2014AJ....147..131P|arxiv=1403.5461|s2cid=119239041}} in the constellation Andromeda. The galaxy was discovered by astronomer by Heinrich d'Arrest on September 16, 1865{{Cite web|url=https://cseligman.com/text/atlas/ngc7a.htm#753|title=New General Catalog Objects: NGC 750 - 799|website=cseligman.com|access-date=2019-01-03}} and is a member of Abell 262.{{Cite journal|last1=Henry|first1=R. B. C.|last2=Balkowski|first2=C.|last3=Cayatte|first3=V.|last4=Edmunds|first4=M. G.|last5=Pagel|first5=B. E. J.|date=1996-12-01|title=The effects of cluster environment on the chemical evolution of galaxies. III. NGC 753.|journal=Monthly Notices of the Royal Astronomical Society|volume=283|issue=2|pages=635–647|doi=10.1093/mnras/283.2.635|issn=0035-8711|bibcode=1996MNRAS.283..635H|doi-access=free}}{{Cite journal|last1=Giuricin|first1=G.|last2=Marinoni|first2=C.|last3=Ceriani|first3=L.|last4=Pisani|first4=A.|date=November 2000|title=Nearby Optical Galaxies: Selection of the Sample and Identification of Groups|journal=The Astrophysical Journal|volume=543|issue=1|pages=178–194|doi=10.1086/317070|issn=0004-637X|arxiv=astro-ph/0001140|bibcode=2000ApJ...543..178G|s2cid=9618325}}{{Cite journal|last=Garcia|first=A. M.|date=1993-07-01|title=General study of group membership. II - Determination of nearby groups|journal=Astronomy and Astrophysics Supplement Series|volume=100|pages=47–90|issn=0365-0138|bibcode=1993A&AS..100...47G}}{{Cite journal|last1=Fouque|first1=P.|last2=Gourgoulhon|first2=E.|last3=Chamaraux|first3=P.|last4=Paturel|first4=G.|date=1992-05-01|title=Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members|journal=Astronomy and Astrophysics Supplement Series|volume=93|pages=211–233|issn=0365-0138|bibcode=1992A&AS...93..211F}}{{Cite web|url=http://simbad.u-strasbg.fr/simbad/|title=NGC 753|website=sim-id|access-date=2019-01-03}}{{Cite web|url=http://ned.ipac.caltech.edu/cgi-bin/NEDatt?objname=NGC+0753|title=Detailed Object Classifications|website=ned.ipac.caltech.edu|access-date=2019-01-03}}

NGC 753 has roughly 2-3 times more mass than the Milky Way and is classified as a radio galaxy.{{Cite journal|last1=Righetti|first1=G.|last2=Giovannini|first2=G.|last3=Feretti|first3=L.|date=1988-04-01|title=WSRT observations at 327 MHz of the cluster A262|journal=Astronomy and Astrophysics Supplement Series|volume=73|pages=173–179|issn=0365-0138|bibcode=1988A&AS...73..173R}}{{Cite journal|last1=Zhao|first1=Jun-Hui|last2=Burns|first2=Jack O.|last3=Owen|first3=Frazer N.|date=1989-07-01|title=A 20 CM VLA survey of Abell clusters of galaxies. I - Distance class of not greater than 3 clusters|journal=The Astronomical Journal|volume=98|pages=64–107|doi=10.1086/115128|issn=0004-6256|bibcode=1989AJ.....98...64Z|doi-access=free}}{{Cite journal|last1=Miller|first1=Neal A.|last2=Owen|first2=Frazer N.|date=2001-06-01|title=The Radio Galaxy Populations of Nearby Northern Abell Clusters|journal=The Astrophysical Journal Supplement Series|volume=134|issue=2|pages=355–383|doi=10.1086/320857|issn=0067-0049|bibcode=2001ApJS..134..355M|arxiv=astro-ph/0101114|s2cid=119052072}}